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Fig. 8


Example of trapping of a s = 10 km planetesimal in a 10/1 mean-motion resonance with the secondary star of γ-Cephei, due to a nonlinear gas drag. Although the orbital migration is divergent, capture still occurs and leads to an apparently stable configuration. The resonant angle is θ = 10λB − λ − 9ϖB.

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